ORBi: Gosset Eric - CPD - 59 deg 2857 - A new red variable star

Reference : CPD - 59 deg 2857 - A new red variable star


	Document type :	Scientific journals : Article
	Discipline(s) :	Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
	To cite this reference:	http://hdl.handle.net/2268/28037

Title :	CPD - 59 deg 2857 - A new red variable star
Language :	English
Author, co-author :	Gosset, Eric [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Groupe d'astrophysique des hautes énergies (GAPHE) >]
	Hutsemekers, Damien [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS) >]
	Surdej, Jean [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS) >]
Publication date :	1985
Journal title :	Publications of the Astronomical Society of the Pacific [=PASP]
Publisher :	University of Chicago Press
Volume :	97
Pages :	67-71
Peer reviewed :	Yes (verified by ORBi)
Audience :	International
ISSN :	0004-6280
	1538-3873
City :	Chicago
Country :	USA
Keywords :	[en] LATE STARS ; LIGHT CURVE ; PECULIAR STARS ; RED GIANT STARS ; STELLAR SPECTRA ; VARIABLE STARS ; EMISSION SPECTRA ; SEMIREGULAR VARIABLE STARS ; STELLAR SPECTROPHOTOMETRY ; UBV SPECTRA
Abstract :	[en] Two (C3 and C4) of the four comparison stars monitored during the photometric study of the peculiar emission-line star GG Car (Gosset et al., 1984) have been found to be variable. Available photometric and spectroscopic data allow us to identify C4 with CPD - 59 deg 2857 and classify it as a late-type giant (M3-4 III) belonging to the red variable stars of the semiregular or irregular type.
Target :	Researchers ; Professionals
Permalink :	http://hdl.handle.net/2268/28037
DOI :	10.1086/131498
Other URL :	http://adsabs.harvard.edu/abs/1985PASP...97...67G
Mentions required by the publisher for OA :	The authors thank SAO/NASA ADS Astronomy Abstract Service for their deposit authorization.

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